Universal power-law distribution functions in an electromagnetic kinetic plasma: implications for the inverted temperature profile in the solar corona
Uddipan Banik, Amitava Bhattacharjee

TL;DR
This paper presents a self-consistent theory showing that electromagnetic turbulence in plasmas leads to universal power-law tails in particle distributions, explaining the inverted temperature profile observed in the solar corona.
Contribution
It introduces a novel quasilinear framework demonstrating universal $v^{-5}$ tails in plasma particle distributions, with implications for solar corona phenomena.
Findings
Electromagnetic turbulence induces universal power-law tails in plasma distributions.
The non-thermal tail facilitates suprathermal particle escape from the sun.
Inversion of the temperature profile in the solar corona is explained by this mechanism.
Abstract
We develop a self-consistent quasilinear theory for the relaxation of electromagnetic kinetic plasmas, and demonstrate that the mean distribution functions of both electrons and ions tend to relax to a universal tail. Large-scale electromagnetic (EM) fields efficiently accelerate the unscreened, fast particles but not the screened, slow ones. This non-thermal tail may arise in the solar corona from EM turbulence despite collisions, allowing suprathermal particles to escape the sun's gravity (velocity filtration) and inverting the temperature profile with rising to K.
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Taxonomy
TopicsSolar and Space Plasma Dynamics · Dust and Plasma Wave Phenomena · Ionosphere and magnetosphere dynamics
